Activity 1: Drawing or Illustration Draw or illustrate Kepler's Three Laws of Motion. Label and explain each illustration. Include the equation used to describe Kepler's Laws of Planetary Motion. Kepler's First Law of Planetary Kepler's Second Law of Motion: Planetary Motion: Drawing/ Illustration Drawing/ Illustration Equation: Explanation: Equation: Explanation: Kepler's Third Law of Planetary Motion: Drawing/ Illustration Equation: Explanation:
Activity 1: Drawing or Illustration Draw or illustrate Kepler's Three Laws of Motion. Label and explain each illustration. Include the equation used to describe Kepler's Laws of Planetary Motion. Kepler's First Law of Planetary Kepler's Second Law of Motion: Planetary Motion: Drawing/ Illustration Drawing/ Illustration Equation: Explanation: Equation: Explanation: Kepler's Third Law of Planetary Motion: Drawing/ Illustration Equation: Explanation:
College Physics
11th Edition
ISBN:9781305952300
Author:Raymond A. Serway, Chris Vuille
Publisher:Raymond A. Serway, Chris Vuille
Chapter1: Units, Trigonometry. And Vectors
Section: Chapter Questions
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![Activity 1: Drawing or Illustration
Draw or illustrate Kepler's Three Laws of Motion. Label and
explain each illustration. Include the equation used to describe
Kepler's Laws of Planetary Motion.
Kepler's First Law of Planetary Kepler's Second Law of
Motion:
Planetary Motion:
Drawing/ Illustration
Drawing/Illustration
Equation:
Explanation:
Equation:
Explanation:
Kepler's Third Law of Planetary
Motion:
Drawing/ Illustration
Equation:
Explanation:
Activity 3: Problem Solving Activity
Answer the following problems and show your process using the
four guide steps for solving problems.
a. The mean solar distance of Earth is 1.50 x m with a period of
1 year. What is the distance of mars from the sun if it has a
period of 1.88 years?
-
b. Titan, the largest moon of Saturn, has a mean orbital radius of
1.22x109 m. The orbital period of Titan is 15.95 days.
Hyperion, another moon of Saturn, orbits at a mean radius of
1.48x109 m. Use Kepler's third law of planetary motion to
predict the orbital period of Hyperion in days.](/v2/_next/image?url=https%3A%2F%2Fcontent.bartleby.com%2Fqna-images%2Fquestion%2F46dfb870-6fdd-4cea-8de9-f7d569cee894%2Fbc8b8023-32d7-453d-881c-8d651586be1f%2Fs1n1acc_processed.jpeg&w=3840&q=75)
Transcribed Image Text:Activity 1: Drawing or Illustration
Draw or illustrate Kepler's Three Laws of Motion. Label and
explain each illustration. Include the equation used to describe
Kepler's Laws of Planetary Motion.
Kepler's First Law of Planetary Kepler's Second Law of
Motion:
Planetary Motion:
Drawing/ Illustration
Drawing/Illustration
Equation:
Explanation:
Equation:
Explanation:
Kepler's Third Law of Planetary
Motion:
Drawing/ Illustration
Equation:
Explanation:
Activity 3: Problem Solving Activity
Answer the following problems and show your process using the
four guide steps for solving problems.
a. The mean solar distance of Earth is 1.50 x m with a period of
1 year. What is the distance of mars from the sun if it has a
period of 1.88 years?
-
b. Titan, the largest moon of Saturn, has a mean orbital radius of
1.22x109 m. The orbital period of Titan is 15.95 days.
Hyperion, another moon of Saturn, orbits at a mean radius of
1.48x109 m. Use Kepler's third law of planetary motion to
predict the orbital period of Hyperion in days.
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